Fundamental Parameters and Spectral Variations of HD 85567
Abstract
We report the results of a spectroscopic study of the emission-line star HD 85567. We refined its fundamental parameters and concluded that it is not a pre-main-sequence star but rather a more evolved FS CMa type object.
- Publication:
-
The B[e] Phenomenon: Forty Years of Studies
- Pub Date:
- February 2017
- Bibcode:
- 2017ASPC..508..377K